Non-LTE Modeling and Observations of Oscillating Prominences
Abstract
Prominence oscillations have been mostly detected using Doppler velocity, although there are also claimed detections by means of the periodic variations of half-width or line intensity. Our main aim here is to explore the relationship between spectral indicators such as Doppler shift, line intensity and line half-width and the linear perturbations excited in a simple prominence model.
- Publication:
-
Nature of Prominences and their Role in Space Weather
- Pub Date:
- January 2014
- DOI:
- 10.1017/S1743921313010740
- Bibcode:
- 2014IAUS..300...52Z
- Keywords:
-
- Sun: oscillations;
- Sun: filaments;
- Sun: prominences